Multi-messenger astrophysics combines multifrequency astronomy in the electromagnetic domain with non photonic information carriers, gravitational waves, neutrinos, cosmic rays, to provide complementary information about cosmic sources. The present paper reviews the recent developments in the instrumentation and the first results of multi-messenger astronomy: the detection of a binary neutron star merger and of high energy neutrinos from a cosmic source.
Late submission of the contribution at Frontier Research in Astrophysics - III (FRAPWS2018)
Volume 362 -
Multifrequency Behaviour of High Energy Cosmic Sources - XIII (MULTIF2019) -
Ongoing Experiments
High Energy Astrophysical Techniques
Full text:
pdf
Pre-published on:
November 23, 2020
Published on:
December 03, 2020
Abstract
DOI: https://doi.org/10.22323/1.362.0082
How to cite
Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in "proceeding" format which is more detailed and complete.
Open Access
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.